Corpotare GS040.2+00.6−70 located on the outskirts of the disk of the milky Way.
Astrophysics from South Korea, USA and Canada explained the origin of the milky Way large sverhusiliya GS040.2+00.6−70 — the rarefied area of irregular shape filled with a heated neutral hydrogen.
The study is published on the website arXiv.org.
Object GS040.2+00.6−70 consists of several clouds. One of them, HVC040+01-282, is located in the center corposana and, as shown by research scientists, with about one hundred kilometers per second departs from it. This allows to clarify the nature of the cloud and the formation of corposana.
Most likely HVC040+01-282 arose about five million years ago in the collision of a fragment of a neighboring galaxy or of intergalactic clouds with the disk of the milky Way. This, scientists believe, led to the formation of corposana.
Another scenario for the appearance of objects of type HVC040+01-282, which the authors do not adhere to in their work, in the birth clouds because of the impact of stellar wind or supernova explosions in stellar associations, located in the molecular clouds and consisting of the stars of spectral classes O or B.
Corpotare GS040.2+00.6−70 located on the outskirts of the disk of the milky Way stretches over a distance of about a kiloparsec. The study of astronomers shows that compact gas clouds moving with high velocities, can migrate through the halo of the milky Way and reach his drive.
